Now that we ve examined the nature of light, let s turn our attention
|
|
- Louise Hines
- 6 years ago
- Views:
Transcription
1 Section Tools for Studying Space 1 FOCUS Section Objectives 24.4 Explain how refracting, reflecting, and radio telescopes work Describe the advantages and disadvantages of each type of 24.6 Explain the advantages that a space telescope has over an Earth-based Key Concepts How does a refracting telescope produce an image? Why are most large telescopes reflecting telescopes? How does a radio telescope gather data? What advantages do space telescopes have over Earthbased telescopes? Vocabulary refracting telescope chromatic aberration reflecting telescope radio telescope Reading Strategy Comparing and Contrasting Copy the Venn diagram. As you read, complete it to show the differences between refracting and reflecting telescopes. Refracting Telescopes Reflecting Telescopes a.? light-gathering, resolving, and b.? magnifying power Reading Focus Build Vocabulary Concept Map Have students make a concept map using the term telescopes as the starting point. All the vocabulary terms in this section should be used. Reading Strategy a. uses a lens to bend and redirect light to a focal point behind a mirror b. uses a concave mirror to focus light to a point in front of a mirror 2 INSTRUCT Refracting Telescopes Build Reading Literacy L1 Refer to p. 642D in Chapter 23, which provides the guidelines for comparing and contrasting. Compare and Contrast Have students read the section. As they read, they should create lists of how the various types of telescopes are similar and different. Verbal Figure 5 Keck Telescope This optical telescope is located at the summit of Hawaii s Mauna Kea volcano. 678 Chapter 24 Now that we ve examined the nature of light, let s turn our attention to the tools astronomers use to intercept and study the energy emitted by distant objects in the universe. Because the basic principles of detecting radiation were originally developed through visual observations, the astronomical tools we ll explore first will be optical telescopes. An example is shown in Figure 5. The 10-meter Keck Telescope, located on Mauna Kea in Hawaii, uses a mosaic of 36 sixsided, 1.8-meter mirrors. The mirrors are carefully positioned by a computer to give the optical effect of a 10-meter mirror. The Keck Telescope is a type of optical To create an image that is a great distance away, a telescope must collect as much light as possible. Optical telescopes contain mirrors, lenses, or both to accomplish this task. Refracting Telescopes Galileo is considered to be the first person to have used telescopes for astronomical observations. Having learned about the newly invented instrument, Galileo built one of his own that was capable of magnifying objects 30 times. Because this early instrument, as well as its modern counterparts, used a lens to bend or refract light, it is known as a refracting 678 Chapter 24
2 Focus The most important lens in a refracting telescope, the objective lens, produces an image by bending light from a distant object so that the light converges at an area called the focus (focus central point). For an object such as a star, the image appears as a point of light. For nearby objects it appears as an inverted replica of the original. You can easily demonstrate the latter case by holding a lens in one hand and, with the other hand, placing a white card behind the lens. Now vary the distance between them until an image appears on the card. The distance between the focus (where the image appears) and the lens is called the focal length of the lens. Astronomers usually study an image from a telescope by first photographing the image. However, if a telescope is used to examine an image directly, a second lens, called an eyepiece, is required. The eyepiece magnifies the image produced by the objective lens. In this respect, it is similar to a magnifying glass. The objective lens produces a very small, bright image of an object, and the eyepiece enlarges the image so that details can be seen. Figure 6 shows the parts of a refracting Objective lens Focal length of objective Focus Focal length of eyepiece Eyepiece Chromatic Aberration Although used extensively in the nineteenth century, refracting telescopes suffer a major optical defect. As light passes through any lens, the shorter wavelengths of light are bent more than the longer wavelengths. Consequently, when a refracting telescope is in focus for red light, blue and violet light are out of focus. The troublesome effect, known as chromatic (chroma color) aberration (aberrare to go astray), weakens the image and produces a halo of color around it. When blue light is in focus, a reddish halo appears. When red light is in focus, a bluish halo appears. Although this effect cannot be eliminated completely, it is reduced by using a second lens made of a different type of glass. Figure 6 Simple Refracting Telescope A refracting telescope uses a lens to bend light. Use Community Resources Invite an astronomer to talk to your class about telescopes. Ask if he or she could bring small telescopes to use for demonstrations. If possible, see if the astronomer could come at night and have a moon-gazing or star-gazing party. Verbal, Interpersonal Making a Simple Refracting Telescope Purpose Students will observe the simple concepts behind a refracting Materials 2 magnifying lenses Procedure Observe an object in the distance with one of the magnifying lenses. Move the lens back and forth until you get a sharp image. Place the second magnifying lens in front of your eye. Move the second lens back and forth until you get a clear image. The image should appear larger. Pass the lenses around the classroom to give students an opportunity to view an image. Expected Outcome Students will see that a simple refracting telescope consists of two lenses. In this example, it consists of two convex lenses. A convex lens is thicker in the middle and thinner around the edges. Visual, Kinesthetic What is chromatic aberration? Studying the Sun 679 Customize for Inclusion Students Learning Disabled For students with difficulty absorbing concepts by reading, use Figures 6, 7, and 8 as a visual aid as you describe how each of these telescopes work. Be sure students understand the differences in these telescopes. Answer to... Chromatic aberration is a troublesome effect associated with refracting telescopes that weakens an image and produces a halo of color around it. Studying the Sun 679
3 Section 24.2 (continued) Reflecting Telescopes Use Visuals L1 Figure 7 Have students examine the figure. Ask: Where is the viewer positioned for each type of reflecting telescope? (In A, the viewer is in a viewing cage inside the telescope, positioned at the focal point. In B, the viewer is seated below the telescope at the focal point. In C, the viewer is at the side of the telescope, viewing the image at an angle.) Infer why the prime focus method is used only for large telescopes. (The telescope has to be large for a person to sit inside the telescope to view the image.) Verbal, Logical Students may think that increasing the magnification of a reflecting telescope will improve the clarity of an image. This is not necessarily true. What can be viewed telescopically is limited by atmospheric conditions and the resolving power of the Any part of an image that is not clear at low magnification will appear only as a larger blur at higher magnification. Increasing magnification spreads out the light and decreases the brightness of the object. Astronomers describe telescopes not in terms of their magnification, but by the diameter of the objective mirror or lens, because it is this factor that determines both the light-gathering power and the resolving power of a A good rule of thumb for amateur astronomers is that for every inch of aperture you can use up to 60 power. A three inch telescope would have a useful magnification of 180. Verbal Figure 7 Viewing Methods with Reflecting Telescopes A The prime method is only used with very large telescopes. B The Cassegrain method is most commonly used. Note that a small hole in the center of the mirror allows light to pass through. C This figure shows the Newtonian method. 680 Chapter 24 A Prime method C For: Links on telescopes Visit: Web Code: cjn-7242 B Cassegrain method Newtonian method Reflecting Telescopes Newton was bothered by chromatic aberration so he built telescopes that reflected light from a shiny surface a mirror. Because reflected light is not dispersed into its component colors, the chromatic aberration is avoided. Reflecting telescopes use a concave mirror that focuses the light in front of a mirror, rather than behind it, like a lens. The mirror is generally made of glass that is finely ground and coated with a highly reflective material, usually an aluminum compound. Because the focus of a reflecting telescope is in front of the mirror, an observer must be able to view the image without blocking too much incoming light. Figure 7A shows a viewing cage for the observer within the Figures 7B and 7C show that the observer can remain indoors. Most large telescopes employ more than one type. Advantages of Reflecting Telescopes As you might guess, it s a huge task to produce a large piece of high-quality, bubblefree glass for refracting telescopes. Most large optical telescopes are reflectors. Light does not pass through a mirror so the glass for a reflecting telescope does not have to be of optical quality. In addition, a lens can be supported only around the edge, so it sags. Mirrors, on the other hand, can be supported fully from behind. One disadvantage of reflecting telescopes is that the secondary mirror blocks some light entering the Thus, a reflecting telescope with a 10- inch opening will not collect as much light as a 10-inch refractor. Properties of Optical Telescopes Both refracting and reflecting telescopes have three properties that aid astronomers in their work: 1) light-gathering power, 2) resolving power, and 3) magnifying power. Light-gathering power refers to the telescope s ability to intercept more light from distant objects, thereby producing brighter images. Telescopes with large lenses or mirrors see farther into space than do those with small ones. Another advantage of telescopes with large objectives is their greater resolving power, which allows for sharper images and finer detail. For example, with the naked eye, the Milky Way appears as a vague band of light in the night sky. But even a small telescope is capable of resolving, or separating it into, individual stars. Lastly, telescopes have magnifying power, which is the ability to make an object larger. Magnification is calculated by dividing the focal length of the objective by the focal length of the eyepiece. Thus, the magnification of a telescope can be changed by simply changing the eyepiece. What is light-gathering power? Download a worksheet on telescopes for students to complete, and find additional teacher support from NSTA SciLinks. 680 Chapter 24
4 A Radio Telescopes Detecting Invisible Radiation As you learned earlier, sunlight is made up of more than just the radiation that is visible to our eyes. Gamma rays, X-rays, ultraviolet radiation, infrared radiation, and radio waves are also produced by stars. Photographic film that is sensitive to ultraviolet and infrared radiation has been developed. This extends the limits of our vision. However, most of this radiation cannot penetrate our atmosphere, so balloons, rockets, and satellites must transport cameras above the atmosphere to record it. A narrow band of radio waves is able to penetrate the atmosphere. Measurement of this radiation is important because we can map the galactic distribution of hydrogen. Hydrogen is the main material from which stars are made. Radio Telescopes The detection of radio waves is accomplished by big dishes called radio telescopes, shown in Figure 8A. In principle, the dish of one of these telescopes operates in the same manner as the mirror of an optical A radio telescope focuses the incoming radio waves on an antenna, which absorbs and transmits these waves to an amplifier, just like a radio antenna. Because radio waves are about 100,000 times longer than visible radiation, the surface of the dish doesn t need to be as smooth as a mirror. Except for the shortest radio waves, a wire mesh is a good reflector. However, because radio signals from celestial sources are very weak, large dishes are necessary to intercept an adequate signal. Radio telescopes have poor resolution, making it difficult to pinpoint the radio source. Pairs or groups of telescopes reduce this problem. When several radio telescopes are wired together, as shown in Figure 8B, the resulting network is called a radio interferometer. B Figure 8 A The 43-meter Radio Telescope at Green Bank, West Virginia The dish acts like the mirror of a reflecting telescope, focusing radio waves onto the antenna. B The Very Large Array Near Socorro, New Mexico Twenty-seven identical antennas operate together to form this radio network. Identifying What is a network of radio telescopes called? Detecting Invisible Radiation Build Science Skills Inferring Explain to students that radio waves are able to penetrate Earth s atmosphere and are used to map the distribution of hydrogen in the galaxy. Ask: The largest radio telescope is 300 m (1,000 ft) in diameter. Why is a radio telescope this large an advantage? (Radio signals from celestial sources are very weak. This telescope is able to collect a larger number of signals because of its size.) This radio telescope was built in a depression in the landscape. Why was this location chosen? (This depression blocks humanmade radio signals from the ) Verbal, Logical Studying the Sun 681 Facts and Figures The Very Large Array consists of 27 radio antennas set up in a Y-shaped configuration. The site is located on the Plains of San Augustin 50 miles west of Socorro, New Mexico. Each antenna measures 25 m in diameter. When the antennas are combined electronically, they give an equivalent resolution of an antenna 36 km in diameter. The combination of the antennas has the sensitivity of a dish that is 130 m in diameter. Answer to... Figure 8 a radio interferometer Light-gathering power refers to the telescope s ability to intercept more light from distant objects, thereby producing brighter images. Studying the Sun 681
5 Section 24.2 (continued) Space Telescopes Integrate Language Arts The Hubble Space Telescope The Hubble Space Telescope has provided spectacular images of the universe. This program also has experienced failures. Have students in groups research the Hubble Space Telescope project and create a computer presentation to share with their classmates. The Internet contains many photographs that can be included in the presentation. Verbal, Interpersonal Q Why do astronomers build observatories on mountaintops? A Observatories are most often located on mountaintops because sites above the densest part of the atmosphere provide better conditions for seeing. Advantages of Radio Telescopes Radio telescopes have some advantages over optical telescopes. They are much less affected by turbulence in the atmosphere, clouds, and the weather. No protective dome is required, which reduces the cost of construction. Viewing is possible 24 hours a day. More important, radio telescopes can see through interstellar dust clouds that obscure visible wavelengths. Radio signals from distant points in the universe pass unhindered through the dust, giving us an unobstructed view. Furthermore, radio telescopes can detect clouds of gases too cool to emit visible light. These cold gas clouds are important because they are the sites of star formation. Radio telescopes are, however, hindered by human-made radio interference. While optical telescopes are placed on remote mountaintops to reduce interference from city lights, radio telescopes are often hidden in valleys to block human-made radio interference. Radio telescopes have revealed such spectacular events as the collision of two galaxies. They led to the important discovery of quasars and pulsars. Why can radio telescopes be used 24 hours a day? Figure 9 Hubble Space Telescope Hubble was deployed into Earth orbit by the space shuttle Discovery. Space Telescopes Have you ever seen a blurring effect caused by the movement of air on a hot summer day? That blurring effect also distorts the images produced by most telescopes on Earth. On a night when the stars twinkle, viewing is difficult because the air is moving rapidly. This causes the image to move about and blur. Observatories are most often located on mountaintops. This is because sites above the densest part of the atmosphere provide better conditions for seeing. At high elevations, there is less air to scatter and dim the incoming light. Also, there is less water vapor to absorb infrared radiation. Further, the thin air on mountaintops causes less distortion of the images being observed. There is one other way to get around the distorting effects of Earth s atmosphere send telescopes into space. Space telescopes orbit above Earth s atmosphere and thus produce clearer images than Earth-based telescopes. Hubble Space Telescope The first space telescope, built by NASA, was the Hubble Space Telescope, shown in Figure 9. Hubble was put into orbit around Earth in April This 2.4-meter space telescope has 10 billion times more light-gathering power than the human eye. Hubble has given us many spectacular images. For example, the 682 Chapter Chapter 24
6 Hubble Space Telescope has provided images that clearly resolve the separation between Pluto and its moon, Charon. It has also provided data about planets that orbit other stars, the birth of stars, black holes, the age of the universe, and the expansion of the universe. Other Space Telescopes Other types of radiation are also affected by Earth s atmosphere. To study X-rays, NASA uses the Chandra X-Ray Observatory. This space telescope was launched in One of its main missions is to gather data about black holes objects whose gravity is so strong that visible light cannot escape them. Another space telescope, the Compton Gamma-Ray Observatory, was used to study both visible light and gamma rays. In 2011, NASA plans to launch the James Webb Space Telescope to study infrared radiation. As Figure 10 shows, images obtained by different telescopes offer different information about the same object in space in this case, the Milky Way galaxy. By studying all the images together, astronomers obtain a more thorough understanding of the galaxy. Figure 10 Images of the Milky Way Galaxy These images were taken by different types of telescopes, including visible light, X-ray, gamma ray, and infrared. 3 ASSESS Evaluate Understanding Have students write down the following types of telescopes: refracting, reflecting, and radio. Then, have students write down three facts about each Have students share their facts with the class. Reteach Use Figures 6, 7, and 8 to review how each of the these telescopes works. Sample answer: Radio waves can easily pass through Earth s atmosphere. Therefore, there is little advantage in sending a radio telescope into space. L1 Section 24.2 Assessment Reviewing Concepts 1. How does a refracting telescope work? 2. How does a reflecting telescope differ from a refracting telescope? 3. Why are most large telescopes reflecting telescopes? 4. How do radio telescopes gather data? 5. Why do space telescopes obtain clearer images than Earth-based telescopes? Critical Thinking 6. Calculating If a telescope has an objective with a focal length of 50 centimeters and an eyepiece with a focal length of 25 millimeter, what will be the magnification? 7. Applying Concepts Using the numbers from the previous question, would an eyepiece with a greater focal length increase or decrease magnification? Explain. Electromagnetic Radiation Recall the different types of electromagnetic radiation. Based on what you ve learned in this section, would you recommend sending a telescope into space to study radio waves? Why or why not? Studying the Sun 683 Answer to... They do not need visible light to obtain images. Section 24.2 Assessment 1. The objective lens produces an image by bending light from a distant object so that the light converges at an area called the focus. 2. A reflecting telescope uses a concave mirror to produce an image. A refracting telescope uses a lens to bend or refract light. 3. Because light does not pass through a mirror, the glass for a reflecting telescope does not have to be of optical quality. In addition, a lens can be supported only around the edge, so it sags. Mirrors, on the other hand, can be supported fully from behind. 4. A radio telescope focuses the incoming radio waves on an antenna, which absorbs and transmits the waves to an amplifier. 5. Space telescopes orbit above Earth s atmosphere and thus produce clearer images than Earth-based telescopes. 6. Magnification is calculated by dividing the focal length of the objective by the focal length of the eyepiece. In this example, 500 mm 25 mm 20; magnification would be 20 times. 7. An eyepiece with a greater focal length, such as 50 mm, would decrease magnification because 500 mm 50 mm 10 times magnification. Studying the Sun 683
Telescopes. Telescopes Key Concepts. glass
Telescopes Telescopes Key Concepts 1) A refracting telescope uses a lens to gather light; a reflecting telescope uses a mirror. ) The main purposes of a telescope are to gather light and resolve fine detail.
More informationAstronomy. Optics and Telescopes
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Optics and Telescopes - Refraction, lenses and refracting telescopes - Mirrors and reflecting telescopes - Diffraction limit,
More informationMeasuring Light waves
Measuring Light waves We normally measure wavelengths (λ) using nanometers (nm) 1 nm = 10-9 m 400-700 nm Increasing wavelengths (λ)! Visible light has wavelengths between 400-700 nm! To detect other types
More informationChapter 23. Light, Astronomical Observations, and the Sun
Chapter 23 Light, Astronomical Observations, and the Sun The study of light Electromagnetic radiation Visible light is only one small part of an array of energy Electromagnetic radiation includes Gamma
More informationAstronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes
Astronomical Tools Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes Laws of Refraction and Reflection Law of Refraction n 1 sin θ 1
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 24 Studying the Sun 24.1 The Study of Light Electromagnetic Radiation Electromagnetic radiation includes gamma rays, X-rays, ultraviolet light, visible
More informationASTR 2310: Chapter 6
ASTR 231: Chapter 6 Astronomical Detection of Light The Telescope as a Camera Refraction and Reflection Telescopes Quality of Images Astronomical Instruments and Detectors Observations and Photon Counting
More informationChapter 6 Light and Telescopes
Chapter 6 Light and Telescopes Guidepost In the early chapters of this book, you looked at the sky the way ancient astronomers did, with the unaided eye. In chapter 4, you got a glimpse through Galileo
More informationTelescopes, Observatories, Data Collection
Telescopes, Observatories, Data Collection Telescopes 1 Astronomy : observational science only input is the light received different telescopes, different wavelengths of light lab experiments with spectroscopy,
More informationChapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Learning Objectives Upon completing this chapter you should be able to: 1. Classify the
More informationCollecting Light. In a dark-adapted eye, the iris is fully open and the pupil has a diameter of about 7 mm. pupil
Telescopes Collecting Light The simplest means of observing the Universe is the eye. The human eye is sensitive to light with a wavelength of about 400 and 700 nanometers. In a dark-adapted eye, the iris
More informationOptics and Telescope. Chapter Six
Optics and Telescope Chapter Six ASTR 111 003 Fall 2007 Lecture 06 Oct. 09, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15) Chap.
More informationAST 101 Intro to Astronomy: Stars & Galaxies
AST 101 Intro to Astronomy: Stars & Galaxies Telescopes Mauna Kea Observatories, Big Island, HI Imaging with our Eyes pupil allows light to enter the eye lens focuses light to create an image retina detects
More informationWhat are the most important properties of a telescope? Chapter 6 Telescopes: Portals of Discovery. What are the two basic designs of telescopes?
Chapter 6 Telescopes: Portals of Discovery What are the most important properties of a telescope? 1. Light-collecting area: Telescopes with a larger collecting area can gather a greater amount of light
More informationEarth s Atmosphere & Telescopes. Atmospheric Effects
Earth s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth s atmosphere can absorb certain wavelengths of light so much that astronomers
More informationWhy Use a Telescope?
1 Why Use a Telescope? All astronomical objects are distant so a telescope is needed to Gather light -- telescopes sometimes referred to as light buckets Resolve detail Magnify an image (least important
More informationTelescopes: Portals of Discovery Pearson Education, Inc.
Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes and cameras work? The Eye Refraction Incoming light ray Air Glass Refraction is the bending
More informationOptics and Telescopes
Optics and Telescopes Guiding Questions 1. Why is it important that telescopes be large? 2. Why do most modern telescopes use a large mirror rather than a large lens? 3. Why are observatories in such remote
More informationChapter 6 Lecture. The Cosmic Perspective Seventh Edition. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Seventh Edition Telescopes Portals of Discovery Telescopes Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes
More informationIII. ASTRONOMY TOOLS:
III. ASTRONOMY TOOLS: A. Since light is so important to astronomers, they want to collect as much of it as possible from a given object, and quantitatively study it in great detail. 1. Astronomers use
More informationFoundations of Astronomy 13e Seeds. Chapter 6. Light and Telescopes
Foundations of Astronomy 13e Seeds Chapter 6 Light and Telescopes Guidepost In this chapter, you will consider the techniques astronomers use to study the Universe What is light? How do telescopes work?
More informationAstronomy 1 Fall 2016
Astronomy 1 Fall 2016 One person s perspective: Three great events stand at the threshold of the modern age and determine its character: 1) the discovery of America; 2) the Reformation; 3) the invention
More informationTelescopes. Optical Telescope Design. Reflecting Telescope
Telescopes The science of astronomy was revolutionized after the invention of the telescope in the early 17th century Telescopes and detectors have been constantly improved over time in order to look at
More informationChapter 6 Lecture. The Cosmic Perspective. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Telescopes Portals of Discovery 2014 Pearson Education, Inc. Telescopes Portals of Discovery CofC Observatory 6.1 Eyes and Cameras: Everyday Light Sensors Our goals
More informationHow do they work? Chapter 5
Telescopes How do they work? Chapter 5 1. History 2. Lenses & Hardware 3. Reflecting Telescopes 4. Refracting Telescopes History Hans Lippershey Middleburg, Holland invented the refractor telescope in
More informationChapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Tools of the Trade: Telescopes The Powers of a Telescope Collecting Power Bigger telescope,
More informationHow Light Beams Behave. Light and Telescopes Guiding Questions. Telescopes A refracting telescope uses a lens to concentrate incoming light at a focus
Light and Telescopes Guiding Questions 1. Why is it important that telescopes be large? 2. Why do most modern telescopes use a large mirror rather than a large lens? 3. Why are observatories in such remote
More informationLight and Telescopes
Light and Telescopes The key thing to note is that light and matter interact. This can happen in four principal ways: 1) emission a hot object such as the filament in a light bulb emits visible light 2)
More informationChapter 5 Telescopes
Chapter 5 Telescopes Units of Chapter 5 Telescope Design Images and Detectors The Hubble Space Telescope Telescope Size High-Resolution Astronomy Radio Astronomy Interferometry Space-Based Astronomy Full-Spectrum
More informationCoursework Booklet 2
Level 3 Applied Science UNIT 16: Astronomy and Space Science PHYSICS SECTION Coursework Booklet 2 1 P a g e Astronomy and space science Learning aim B Undertake measurement and observation of astronomical
More information2007 Oct 9 Light, Tools of Astronomy Page 1 of 5
Light Waves, Tools of Astronomy I. Vibrations and waves A. Wiggle in time is a vibration needs elapsed time to occur B. Wave is created by vibration exists over space and time C. Types 1. Sound wave needs
More informationUniverse. Chapter 6. Optics and Telescopes 11/16/2014. By reading this chapter, you will learn. Tenth Edition
Roger Freedman Robert Geller William Kaufmann III Universe Tenth Edition Chapter 6 Optics and Telescopes By reading this chapter, you will learn 6 1 How a refracting telescope uses a lens to form an image
More informationLearning aim B: Astronomical measurements and observations
Learning aim B: Astronomical measurements and observations Types of telescopes There are 2 different types of telescopes, each with their own advantages and disadvantages: Reflecting telescopes Refracting
More informationChapter 6 Telescopes: Portals of Discovery. Agenda. How does your eye form an image? Refraction. Example: Refraction at Sunset
Chapter 6 Telescopes: Portals of Discovery Agenda Announce: Read S2 for Thursday Ch. 6 Telescopes 6.1 Eyes and Cameras: Everyday Light Sensors How does your eye form an image? Our goals for learning How
More informationTELESCOPES POWERFUL. Beyond the Book. FOCUS Book
FOCUS Book POWERFUL TELESCOPES Why do we need telescopes in order to observe stars that are very far away? Why do stars look bright in the sky while most galaxies, which have billions of stars, are too
More informationUniverse. Chapter 6. Optics and Telescopes 8/12/2015. By reading this chapter, you will learn. Tenth Edition
Roger Freedman Robert Geller William Kaufmann III Universe Tenth Edition Chapter 6 Optics and Telescopes By reading this chapter, you will learn 6 1 How a refracting telescope uses a lens to form an image
More information1. Using, scientists can use a few smaller telescopes to take images with the. 2. To double the resolving power of a telescope, you must.
Chapter 5 Telescopes Multiple Choice Questions 1. Using, scientists can use a few smaller telescopes to take images with the same resolution as a much larger telescope. A. Satellite telescopes B. Charge-coupled
More informationChapter 24 Studying the Sun
Chapter 24 Studying the Sun Section 1 The Study of Light Key Concepts What types of radiation make up the electromagnetic spectrum? What can scientists learn about a star by studying its spectrum? How
More informationChapter 6 Telescopes: Portals of Discovery
Chapter 6 Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How does your eye form an image? How do we record images? How does your eye form an image?
More informationUniverse Now. 2. Astronomical observations
Universe Now 2. Astronomical observations 2. Introduction to observations Astronomical observations are made in all wavelengths of light. Absorption and emission can reveal different things on different
More informationTools of Modern Astronomy
Tools of Modern Astronomy Are Those Stars Really a Group? 1. Cut ten pieces of thread to different lengths between 5 cm and 25 cm. Tape a 1- cm plastic foam ball to the end of each piece of thread. 2.
More informationTELESCOPES An overview of the main tools used by astronomers to study the universe.
Lesson 203: TELESCOPES An overview of the main tools used by astronomers to study the universe. Fundamental Questions Attempting to give thorough and reasonable answers to the following questions will
More informationPhys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5
Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5 MULTIPLE CHOICE 1. What is the wavelength of the longest wavelength light visible to the human eye? a. 400 nm b. 4000 nm c. 7000 nm
More informationRefraction is the bending of light when it passes from one substance into another. Your eye uses refraction to focus light.
Telescopes Portals of Discovery Chapter 6 Lecture The Cosmic Perspective 6.1 Eyes and Cameras: Everyday Light Sensors How do eyes and cameras work? Seventh Edition Telescopes Portals of Discovery The Eye
More informationProperties of Thermal Radiation
Observing the Universe: Telescopes Astronomy 2020 Lecture 6 Prof. Tom Megeath Today s Lecture: 1. A little more on blackbodies 2. Light, vision, and basic optics 3. Telescopes Properties of Thermal Radiation
More informationLight and motion. = v c
Light and motion This means that if you know what wavelength some radiation was emitted at (as you would for, say, a hydrogen Balmer line), then the observed wavelength tells you the velocity of the object
More informationLight and Telescopes
Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we
More informationCASSEGRAIN TELESCOPE
CASSEGRAIN TELESCOPE ------- Interactive Physics Simulation ------- Page 01 How does a telescope collect and magnify light? We describe the shape of a telescope by its f/#, roughly speaking the ratio of
More informationWriting very large numbers
19.1 Tools of Astronomers Frequently in the news we hear about discoveries that involve space. Since the 1970s, space probes have been sent to all of the planets in the solar system and we have seen them
More informationA stronomers are in the business of gathering and studying light.
24.1 The Study of Light Key Concepts What types of radiation make up the electromagnetic spectrum? What can scientists learn about a star by studying its spectrum? How can astronomers determine whether
More informationOn to Telescopes. Imaging with our Eyes. Telescopes and cameras work much like our eyes. ASTR 1120 General Astronomy: Stars & Galaxies !
ASTR 1120 General Astronomy: Stars & Galaxies On to Telescopes!AST CLASS Learning from light: temperature (from continuum spectrum) chemical composition (from spectral lines) velocity (from Doppler shift)
More informationTelescopes. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. Key Ideas:
Telescopes A Warm Up Exercise If we measure the wavelengths of emission lines and absorption lines from the same gas, we find that (ignoring any Doppler shifts) a) Some emission lines shift to the red
More informationHow does your eye form an Refraction
Astronomical Instruments Eyes and Cameras: Everyday Light Sensors How does your eye form an image? How do we record images? How does your eye form an image? Refraction Refraction is the bending of light
More informationASTR 1120 General Astronomy: Stars & Galaxies
ASTR 1120 General Astronomy: Stars & Galaxies!AST CLASS Learning from light: temperature (from continuum spectrum) chemical composition (from spectral lines) velocity (from Doppler shift) "ODA# Detecting
More informationTelescopes. Lecture 7 2/7/2018
Telescopes Lecture 7 2/7/2018 Tools to measure electromagnetic radiation Three essentials for making a measurement: A device to collect the radiation A method of sorting the radiation A device to detect
More informationAstronomy 1504/15014 Section 20
1 point each Astronomy 1504/15014 Section 20 Midterm 1 (Practice Exam) September 21, 2015 Exam Version A Choose the answer that best completes the question. Read each problem carefully and read through
More informationPHYS 160 Astronomy Test #2 Fall 2017 Version A
PHYS 160 Astronomy Test #2 Fall 2017 Version A I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. A blackbody emits all of its radiation
More informationOptical Telescopes. Telescopes. Refracting/Reflecting Telescopes. Physics 113 Goderya
Telescopes Physics 113 Goderya Chapter(s): 6 Learning Outcomes: Optical Telescopes Astronomers use telescopes to gather more light from astronomical objects. The larger the telescope, the more light it
More informationTWO SMALL PIECES OF GLASS A Space Science Program for Grades 5-12
Teacher Idea Kit TWO SMALL PIECES OF GLASS A Space Science Program for Grades 5-12 Presented by Funded in part by: Two Small Pieces of Glass Suggested for Grades 5-12 Objectives After visiting the planetarium
More informationTelescopes and estimating the distances to astronomical objects
Telescopes and estimating the distances to astronomical objects Why do we use telescopes? 1. Light-collecting area: A telescope is a light bucket Q: How much more light can a telescope with a diameter
More informationAstro 1010 Planetary Astronomy Sample Questions for Exam 3
Astro 1010 Planetary Astronomy Sample Questions for Exam 3 Chapter 6 1. Which of the following statements is false? a) Refraction is the bending of light when it passes from one medium to another. b) Mirrors
More informationChapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization
Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes
More informationTelescopes... Light Buckets
Telescopes... Light Buckets Now that we have an understanding of what light is and why it s important to astronomy, what tools are required to study light from distant objects? The telescope is the tool
More informationFocus Question: How do astronomers study light?
Telescopes Focus Question: How do astronomers study light? Telescopes Tools for collecting and analyzing electromagnetic radiation (light) in ways beyond what we can do with our eyes alone Properties of
More information1) What do all waves transport from one place to another?
Pre Quiz 1) What do all waves transport from one place to another? 2) In which of the following scenarios would the Doppler effect be present? a) A police car, with its siren sounding, speeds past you
More informationAstronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION
Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION CHAPTER 3 Telescopes Lecture Presentation 3.0 Imaging the universe Our original observations of the universe depended on our eyes! What other
More informationTelescopes. Optical Telescope Design. Reflecting Telescope
Telescopes The science of astronomy was revolutionized after the invention of the telescope in the early 17th century Telescopes and detectors have been constantly improved over time in order to look at
More informationTelescopes: Portals of Discovery
Telescopes: Portals of Discovery How do light and matter interact? Emission Absorption Transmission Transparent objects transmit light Opaque objects block (absorb) light Reflection or Scattering Reflection
More informationOptical Telescopes. Not *INVENTED* by Galileo, but he was the first to point it at the sky in 1609.
Telescopes! Optical Telescopes Not *INVENTED* by Galileo, but he was the first to point it at the sky in 1609. The Purpose of a Telescope Gather as much light as possible Reveal as much detail as possible
More informationUNIT E: SPACE EXPLORATION
UNIT E: SPACE EXPLORATION S C I E N C E 9 1 Science 9 Unit E Section 3.0 OPTICAL TELESCOPES, RADIO TELESCOPES, AND OTHER TECHNOLOGIES ADVANCE OUR UNDERSTANDING OF SPACE SECTI ON 3.0 Science 9 Unit E Section
More informationHow does your eye form an Refraction
Astronomical Instruments and : Everyday Light Sensors How does your eye form an image? How do we record images? How does your eye form an image? Refraction Refraction is the of light Eye uses refraction
More information4. Our eyes can only see a small band of the entire spectrum of light. A) True B) False
1. Galileo was able to determine a precise value of the speed of light by using a technique that involved shuttered lanterns and his assistant on a different hill of known distance. 2. According to Einstein's
More informationTools of Astronomy: Telescopes
Tools of Astronomy: Telescopes Lecture 9 1 Refracting Telescopes Large lens to gather and focus light. Incoming Light Objective Lens Focus Eyepiece 2 Problems w/ Refracting Tel s Must make a large piece
More informationASTR-1010: Astronomy I Course Notes Section VI
ASTR-1010: Astronomy I Course Notes Section VI Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
More informationParallel Rays From Distant Objects. 6. Optics and Telescopes. Refraction & Reflection
6. Optics and Telescopes Refracting telescopes Reflecting telescopes Image degradation Imaging systems Spectrographs Non-optical telescopes Orbiting telescopes Parallel Rays From Distant Objects Refracting
More informationDoppler Shifts. Doppler Shift Lecture-Tutorial: Pgs Temperature or Heat? What can we learn from light? Temp: Peak in Thermal Radiation
Doppler Shift Lecture-Tutorial: Pgs. 75-80 Work with a partner or two Read directions and answer all questions carefully. Take time to understand it now! Come to a consensus answer you all agree on before
More informationTelescopes. Some of these are made into satellites and put into the atmosphere
Telescopes Telescopes Telescopes collect more light than the eye can which is why they allow us to see much fainter objects than is possible with the naked eye In the past astronomers look through them,
More informationIt will cover material up to, but not including, Will consist of a few short-answers, 1-2 short essay, and a few problems + extra credit.
Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building This Class (Lecture 13): Thermal Radiation Next Class: Exam #1 on Friday! Thursday Review Session Hour Exam #1 Music: The Space Race is Over
More informationTelescopes. Bởi: OpenStaxCollege
Telescopes Bởi: OpenStaxCollege Telescopes are meant for viewing distant objects, producing an image that is larger than the image that can be seen with the unaided eye. Telescopes gather far more light
More informationEarth based radio telescopes
I am telescope. My purpose is to collect as much light as possible from some distant source and deliver it to a detector/observer for detailed study. Different Telescopes opaque opaque Space based telescopes
More informationHubble Space Telescope
Before the first telescopes were invented at the beginning of the 17th century, people looked up at the stars with their naked eyes. The first refracting telescope that Galileo developed in 1609 was likely
More informationAgenda Announce: Visions of Science Visions of Science Winner
7. Telescopes: Portals of Discovery All of this has been discovered and observed these last days thanks to the telescope that I have [built], after having been enlightened by divine grace. Galileo Galilei
More informationChapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Why do we need Telescopes? Large collection area for photons than the eye long integration
More informationThe Main Point. Familiar Optics. Some Basics. Lecture #8: Astronomical Instruments. Astronomical Instruments:
Lecture #8: Astronomical Instruments Astronomical Instruments: Optics: Lenses and Mirrors. Detectors. Ground Based Telescopes: Optical, Infrared, and Radio. Space Based Telescopes. Spacecraft Missions.
More informationANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study
Stars, Galaxies, a the Universe Stars, Galaxies, and the Universe Telescopes Use Target Reading Skills Check student definitions for accuracy. 1. Electromagneticradiationisenergythatcan travel through
More informationReview. PHYS 162 Lecture 5a 1
Review Light as both wave properties (freq. wavelength) and particle properties (photon is a discrete light unit) Speed of light constant in ALL rest frames time and space accomodates this (Einstein) Wavelength,
More informationLecture 4: Telescopes. Previous Topics.
Lecture 4: Telescopes Web site Stuff from last time Naked eye and magnitudes Development of telescopes Types of telescopes http://www.pa.msu.edu/courses/2003spring/ast312/ This is the class web page. Be
More informationChapter 5. Telescopes. Dr. Tariq Al-Abdullah
Chapter 5 Telescopes The Tools of Astronomy Dr. Tariq Al-Abdullah Learning Goals: 5.1 Optical Telescopes (The Hubble Space Telescope) 5.2 Telescope Size 5.3 Images and Detectors 5.4 High-Resolution Astronomy
More informationPreteach. Target Reading Skill. Build Background Knowledge
Section 1 Telescopes 1 Telescopes Objectives After this lesson, students will be able to J.4.1.1 State the regions of the electromagnetic spectrum. J.4.1.2 Explain what telescopes are and how they work.
More information7. Telescopes: Portals of Discovery Pearson Education Inc., publishing as Addison Wesley
7. Telescopes: Portals of Discovery Parts of the Human Eye pupil allows light to enter the eye lens focuses light to create an image retina detects the light and generates signals which are sent to the
More informationTelescopes. Astronomy 320 Wednesday, February 14, 2018
Telescopes Astronomy 320 Wednesday, February 14, 2018 Telescopes gather light and resolve detail A telescope is sometimes called a light bucket. Number of photons collected per second is proportional to
More informationTelescopes 3 Feb. Purpose
Telescopes 3 Feb Key parameters of telescopes Optical telescopes SOAR Telescope, MSU s window on the universe Radio telescopes Telescopes in space SOAR Telescope Cerro Pachon, Chile First Test is Thurs
More informationABOUT SPOTTINGSCOPES Background on Telescopes
22 November 2010 ABOUT SPOTTINGSCOPES A spotting scope is a compact telescope designed primarily for terrestrial observing and is used in applications which require magnifications beyond the range of a
More informationHow do telescopes "see" on Earth and in space?
How do telescopes "see" on Earth and in space? By NASA, adapted by Newsela staff on 03.28.17 Word Count 933 Level 970L TOP IMAGE: The Hubble Space Telescope orbiting in space over Earth. SECOND IMAGE:
More information~ λ / D. Diffraction Limit 2/7/17. Topics for Today. Problems in Looking Through Our Atmosphere. ASTR 1040: Stars & Galaxies
ASTR 1040: Stars & Galaxies Gran Telescopio Canarias, La Palma 10.4m Topics for Today What our atmosphere does to light Magic of adaptive optics Radio telescopes: many dishes make a big one (interferometry
More informationTelescopes (Chapter 6)
Telescopes (Chapter 6) Based on Chapter 6 This material will be useful for understanding Chapters 7 and 10 on Our planetary system and Jovian planet systems Chapter 5 on Light will be useful for understanding
More informationa. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU
1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy
More informationChapter 5 Light: The Cosmic Messenger. Copyright 2012 Pearson Education, Inc.
Chapter 5 Light: The Cosmic Messenger 5.1 Basic Properties of Light and Matter Our goals for learning: What is light? What is matter? How do light and matter interact? What is light? Light is an electromagnetic
More informationAnnouncements. Topics To Be Covered in this Lecture
Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 3rd LearningCurve activity was due earlier today! Assignment 3 and
More informationAssignments. For Mon. 1 st Midterm is Friday, Oct. 12. Read Ch. 6 Optionally do MT1-sample-problems
Assignments For Mon. Read Ch. 6 Optionally do MT1-sample-problems 1 st Midterm is Friday, Oct. 12 Chapter 5 Light: The Cosmic Messenger Thermal Radiation 1. Hotter objects emit photons with a higher average
More information